Heliophysics Events Knowledgebase Coverage Registry (HCR)
The JSOC server room was significantly affected by flooding on 2024-11-26. JSOC team processes IRIS, AIA, and HMI Level 0 and Level 1 files; those data pipelines will be down until further notice.
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2015-09-02 11:35:21-14:28:55
HOP206 (N pole)
Polar Panorama Map for understanding Polar Reversal in Cycle 24
x,y:-16",881"
Max FOV:316"x162"
Target:Limb, N Pole
Nearby Events
6302A Continuum Intensity316"x162"1008 spectra
6302A Longitudinal Flux Density316"x162"1008 spectra
6302A Transverse Flux Density316"x162"1008 spectra
6302A Velocity 6301.5A316"x162"1008 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 16 MB
SOTSP: HOP206 (N pole)
2015-09-02T11:35:21 to 2015-09-02T14:28:55
Science Goal: Polar Panorama Map for understanding Polar Reversal in Cycle 24
Program: Fast deep mode, 2048 slit position, LIMB ONLY
Target: Limb, N Pole
xcen=-16 ycen=881
Instrument: SOTSP
HOP/JOP: 206
Description: The data obtained by the HOP81 observations show that the longitudinal dependence of polar reversal is large. Especially, the dependence becomes important for understanding the progress of polar reversal when polar reversal is progressing to the final phase. Hence, we propose the special observation for taking the panorama map of magnetic field around Pole. If we want to make the panorama map that covers until 65 degrees latitude, we need to perform the polar observation every 3.5 days during one month. Considering the matters about Hinode operation (flares, satellite operation, etc.), we request to perform the polar observation every 3 days. It means that we need to perform 10 polar observations for one panorama map during one month.

The data obtained by the HOP81 observations show that the longitudinal dependence of polar reversal is large. Especially, the dependence becomes important for understanding the progress of polar reversal when polar reversal is progressing to the final phase. Hence, we propose the special observation for taking the panorama map of magnetic field around Pole. If we want to make the panorama map that covers until 65 degrees latitude, we need to perform the polar observation every 3.5 days during one month. Considering the matters about Hinode operation (flares, satellite operation, etc.), we request to perform the polar observation every 3 days. It means that we need to perform 10 polar observations for one panorama map during one month.

Annotations:
Hits: 61
Chief Observer
DeRosa (RCO)
Related Links
Cites: HOP206 (N pole)     
Timeline: gif use
See also
Datasets
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: -1 min fov: 316,162 images: 1008 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: -1 min fov: 316,162 images: 1008 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: -1 min fov: 316,162 images: 1008 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: -1 min fov: 316,162 images: 1008 JavaScript Landing Page
Time Series (SP Datacubes)